How to Correctly Stitch Together {\it Kepler} Data of a Blazhko Star

D. W. Kurtz; F. Ekmek\c{c}\.i; H. V. \c{S}enavc{\i}; J. M. Benk\H{o}; J. Nemec; K. Kinemuchi; K. Kolenberg; L. \c{C}el\.ik; R. Szab\'o

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How to Correctly Stitch Together {\it Kepler} Data of a Blazhko Star

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arxiv 1202.3607 v1 pith:4MJB6QM2 submitted 2012-02-16 astro-ph.SR

L. Çeli̇k , F. Ekmekçi̇ , J. Nemec , K. Kolenberg , J. M. Benkő , R. Szabó , D. W. Kurtz , K. Kinemuchi

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H. V. Şenavc{i}

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classification astro-ph.SR

keywords blazhkodatakeplerstaranalysisprocessstitchingtogether

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One of the most challenging difficulties that precedes the frequency analysis of {\it Kepler} data for a Blazhko star is stitching together the data from different seasons (quarters). We discuss the preliminary steps in the stitching, detrending and rescaling process using the data for long-term Blazhko stars. We present the process on {\it Kepler} data of a Blazhko star with a variable Blazhko cycle and some first results of our analysis.

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